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Massive Decline of the World's Largest King Penguin Colony at Ile Aux

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Massive Decline of the World's Largest King Penguin Colony at Ile Aux Antarctic Science 30(4), 236–242 (2018) © Antarctic Science Ltd 2018 doi:10.1017/S0954102018000226 Massive decline of the world’s largest king penguin colony at Ile aux Cochons, Crozet HENRI WEIMERSKIRCH1, FABRICE LE BOUARD1,2, PETER G. RYAN3 and C.A. BOST1 1Centre d’Etudes Biologiques Chizé, CNRS – Université de la Rochelle, 79360 Villiers en Bois, France 2Réserve Nationale des Terres Australes Françaises, TAAF, 97420 Saint Pierre, La Réunion 3FitzPatrick Institute of African Ornithology, DST-NRF Centre of Excellence, University of Cape Town, Rondebosch 7701, South Africa [email protected] Abstract: King penguins (Aptenodytes patagonicus Miller) are major consumers in the Southern Ocean. The colony at Ile aux Cochons, Iles Crozet, in the southern Indian Ocean was known in the 1980s as the largest king penguin colony and the second largest penguin colony in the world. However, there have not been any recent estimates of this colony. Aerial photographs taken from a helicopter, and satellite images were used to report on changes in the colony and population sizes over the past 50 years. The colony has declined by 88% over the past 35 years, from c. 500 000 pairs to 60 000 pairs. The possible causes of this decline were explored but no plausible explanation for such an unprecedented decrease in penguin populations was found. The study highlights the use of satellite imagery as a non-invasive technique for population monitoring, and stresses the need for further research on the causes of this alarming trend in this colony. Received 14 December 2017, accepted 23 April 2018 Key words: Aptenodytes patagonicus, satellite image, remote sensing Introduction Tamaris colony accounted for a significant proportion of the total consumption by the seabird community in the King penguins (Aptenodytes patagonicus Miller) are Indian Ocean at this time (Guinet et al. 1996) and was major consumers in the Southern Ocean (Guinet et al. considered to be the second largest penguin colony in the 1996). During the breeding season, they mostly eat world (Convey et al. 1999). The monitoring of this myctophid fish that are caught in deep waters, mainly in immense colony has become a priority for monitoring the Polar Frontal Zone (South Georgia: Scheffer et al. programmes in the Southern Ocean, especially since the (2012), Marion: Pistorius et al. (2017), Crozet: Bost et al. 1997 El-Niño event negatively affected the foraging (2015)). Numbers of king penguins have increased capacities, and as a result the survival and growth rates, throughout the Southern Ocean over the past 50 years of king penguins on nearby Ile de la Possession, 100 km to (Weimerskirch et al. 1989, 1992, Sanders 2006, Crawford the east of Ile aux Cochons (Bost et al. 2015). et al. 2009). This increase has been interpreted as a This paper reports on changes in size over the past 50 recovery from historical exploitation in the 19th century years at Ile aux Cochons. Satellite imagery and recent (Rounsewell & Copson 1982, Weimerskirch et al. 1992) photographs taken from helicopters were used to estimate or change in the functioning of trophic food webs (Guinet the surface area occupied by the colony and to infer et al. 1996). However, their numbers may fluctuate changes in the population size. extensively in response to large-scale climatic events such as the Sub-Tropical Indian Dipole and El-Niño Materials and methods Southern Oscillation (ENSO; Le Bohec et al. 2008, Bost et al. 2015). Until now, the Morne du Tamaris Colony, Ile Ile aux Cochons (67 km2) is one of the three larger islands aux Cochons, Iles Crozet, in the southern Indian Ocean, of the Crozet archipelago located at 46.1°S, 50.2°E. It is a has been known as the largest king penguin colony remote island that is rarely visited. The large king penguin (Guinet et al. 1995). This colony, discovered and colony is located c. 1.5 km from the eastern shore of the photographed by a cartographic team in 1962, was island on the border of an ancient volcanic cone, the estimated from surface measurements of the colony and Morne du Tamaris (144 m, Fig. 1). breeding densities to contain more than 300 000 pairs of King penguins breed in large colonies on flat or gently king penguins (Bauer 1963) (Table I). Later estimates sloping, unvegetated ground, where they are dispersed from satellite images indicated that it had increased in the regularly, at densities of 1.6–2.2 incubating birds per surface area occupied, and hosted c. 500 000 breeding square metre (Bauer 1967, Barrat 1976). Densities of pairs in 1982–1988 (Guinet et al. 1995). The Morne du incubating penguins increase only slightly when the 236 Downloaded from https://www.cambridge.org/core. IP address: 170.106.35.229, on 02 Oct 2021 at 04:50:15, subject to the Cambridge Core terms of use, available at https://www.cambridge.org/core/terms. https://doi.org/10.1017/S0954102018000226 MASSIVE PENGUIN DECLINE 237 Table I. Estimates of colony surface area (bare surfaces), surfaces occupied by breeding king penguins, and number of breeding pairs based on 1.6 incubating individuals per square metre (Bauer 1967), based on oblique photographs taken from a helicopter and satellite imagery, for the Ile aux Cochons colony of Morne du Tamaris. Area occupied by No. of breeding Date Survey method Colony area (m2) breeding pairs (m2) pairs Reference End Dec 1962 Helicopter, vertical 198 000 317 000 Bauer 1967 15 Feb 1982 Helicopter, vertical 314 000 502 400 Institut Géographique National, Guinet et al. 1995 19 Jan 1988 Spot satellite 308 500 494 000 Guinet et al. 1995 24 Jan 2005 WordlView-3 VHR satellite 223 200 20 Jan 2015 WorldView-3 satellite 120 549 47 900 76 640 30 Dec 2016 Helicopter, oblique 50 926 ACE cruise 18 April 2017 WorldView-3 satellite 114 052 37 284 59 200 number of incubating birds in a colony increases, as king Marion Dufresne in December 1999 and from the RS penguins do not build nests, and disperse, slightly more Akademik Tryoshnikov on 30 December 2016 during the than one flipper length apart (Barrat 1976). Laying starts Antarctic Circumpolar Expedition (ACE; PGR, FL). In in mid-November, with peak numbers of breeding birds addition, high-resolution multispectral satellite images being observed in January (Weimerskirch et al. 1992, taken in January 2015 and April 2017 from the Descamp et al. 2002). WorldView-3 VHR satellite were used, with the visible Published (Bauer 1967, Guinet et al. 1995) and more bands (2/3/5) pan-sharpened to provide 31-cm resolution recent oblique photographs taken from helicopters, and colour images from Digital Globe (https://www. satellite images, were compiled (Table I). In addition to digitalglobe.com) (Table I). helicopter flights over the Morne du Tamaris colony in From satellite images it can be seen that breeding 1962 and 1982, flights were carried out from the RS ‘patches’ occur in bare areas, clearly distinguishable from Fig. 1. Satellite images of the Morne du Tamaris king penguin colony at different scales. Downloaded from https://www.cambridge.org/core. IP address: 170.106.35.229, on 02 Oct 2021 at 04:50:15, subject to the Cambridge Core terms of use, available at https://www.cambridge.org/core/terms. https://doi.org/10.1017/S0954102018000226 238 HENRI WEIMERSKIRCH et al. surrounding vegetated areas (Fig. 1). The surface area of surfaces have shrunk by 64% from their maximum extent the bare ground can be used to estimate the surface area in 1982 to a minimum in 2017 (Table I). The total surface occupied by the colony, provided that breeding birds area has decreased progressively since 1982, as shown by occupy the entire bare ground (Guinet et al. 1995). surface contour lines in Fig. 2. Recent satellite images However, during recent years, even at peak breeding time show that a large section of the former maximum surface in January, nesting birds have not occupied the entire has been re-vegetated rapidly over the last 10 years. surface area of bare ground (Fig. 1). Thus when possible, When peak numbers of incubating birds were present with the most recent high-resolution satellite images from the colony occupied only 40% of the surface available in 2015 and 2017, both the entire bare surface area and the January 2015, and 32% in April 2017, when adult birds surface area occupied by breeding penguins were estimated. were brooding late chicks, and large chicks were grouped Surfaces were estimated by importing satellite images into in crèches. Oblique photographs taken by helicopter the Quantum GIS geographical information system and confirmed that the colony was occupying a reduced area outlining the border of the surfaces. The number of of bare ground. The 2015 data are considered for breeders was estimated by using the conservative figure of comparison with historical counts because this was the 1.6 pairs per square metre (Bauer 1967). period of maximum occupancy of the colony, and the images obtained in 2015 clearly distinguish areas of bare ground from the areas occupied by incubating birds Results (Table I, Fig. 3). The data from April 2017 cannot be used A comparison of estimates of the total surface area in the comparison with historical counts, as most of the occupied by the colony of Morne du Tamaris between breeders at this time had left their chicks unattended in 1962 and 2017 indicates that areas of bare and occupied crèches (Barrat 1976). Thus, considering that the colony Fig. 2. Contours of the extent of the king penguin colony in 1982 (total bare ground occupied by breeders), 2005 (bare ground) and 2015 (bare ground), applied on the 2015 satellite image.
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